activity
20072026
most citedPhysics of Solar Prominences: II - Magnetic Structure and Dynamics

631 citations · 4.6k across the 88 of their papers we have counts for

collaborators

90 papers

astro-ph.SR2026

Magnetohydrodynamic coronal modelling with high-fidelity magnetograms

Haopeng Wang, Stefaan Poedts, Wensi Wang +16

To resolve coronal structures in detail, it is essential to constrain the coronal model using high-fidelity magnetograms with minimal smoothing. In this paper, we improve the numer…

astro-ph.SR2026

Supersonic flows observed by THEMIS related to a coronal bright point and filament

Garima Karki, Brigitte Schmieder, Ramesh Chandra +3

In this paper, we report on the dynamics of the fine structure of a solar quiescent filament observed on September 28, 2023, with the Télescope Héliographique pour l'Etude du Magné…

astro-ph.SR2023★ 4 cited

Two-horn quiescent prominence observed in H-alpha and MgII h&k lines with THEMIS and IRIS

Krzysztof Barczynski, Brigitte Schmieder, Bernard Gelly +2

Prominences are large magnetic structures in the corona filled by cool plasma with fast evolving fine structure. We aim to better understand the plasma conditions in the fine struc…

astro-ph.SR2023

Understanding the Lateral Drifting of an Erupting Filament with a Data-constrained Magnetohydrodynamic Simulation

Jinhan Guo, Ye Qiu, Yiwei Ni +6

Solar filaments often exhibit rotation and deflection during eruptions, which would significantly affect the geoeffectiveness of the corresponding coronal mass ejections (CMEs). Th…

astro-ph.SR2023

Impact of the solar activity on the propagation of ICMEs: Simulations of hydro, magnetic and median ICMEs at minimum and maximum of activity

Barbara Perri, Brigitte Schmieder, Pascal Démoulin +2

The propagation of Interplanetary Coronal Mass Ejections (ICMEs) in the heliosphere is influenced by many physical phenomena, related to the internal structure of the ICME and its…

astro-ph.SR2023★ 24 cited

Rotation and interaction of the September 8 and 10, 2014 CMEs tested with EUHFORIA

Anwesha Maharana, Camilla Scolini, Brigitte Schmieder +1

Solar coronal mass ejections (CMEs) can catch up and interact with preceding CMEs and solar wind structures to undergo rotation and deflection during their propagation. We aim to s…